Charge-independent trend of isoscalar matrix elements along the $N \sim Z$ line

dc.creatorOrce, J. N.
dc.creatorVelazquez, V.
dc.date2006-03-09
dc.date.accessioned2026-07-07T07:07:32Z
dc.date.available2026-07-07T07:07:32Z
dc.descriptionShell model calculations have been carried out using the m-scheme numerical code {\small ANTOINE} in order to elucidate the particular trend of the isoscalar matrix elements, $M_0$, for $A=4n+2$ isobaric triplets ranging from A=18 to A=42. The 2${_1^+}_{(T=1)}$ $\to$ 0${_1^+}_{(T=1)}$ transition energies, reduced transition probabilities and isoscalar matrix elements are predicted to a high degree of accuracy. The general agreement of $M_0$ between those from mirror pairs and those from $T_Z=0$ nuclides support our shell model calculations. The predicted results tie together recent experimental data, and the trend of $M_0$ strength along the $sd$ and beginning of the $fp$ shells is interpreted in terms of the dynamic shell structure. Certain discrepancies arise at A=18 and A=38 isobaric triplets, which might be explained in terms of core polarization effects and the low occupancy of the orbits at the extremes of the $sd$ shell.
dc.description7 pages, 3 figs
dc.identifierhttps://arxiv.org/abs/nucl-th/0603030
dc.identifierhttp://arxiv.org/abs/nucl-th/0603030
dc.identifierNucl.Phys. A764 (2006) 205-211
dc.identifierdoi:10.1016/j.nuclphysa.2005.09.023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/110427
dc.subjectNuclear Theory
dc.titleCharge-independent trend of isoscalar matrix elements along the $N \sim Z$ line
dc.typetext

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